「宇宙の間欠泉」から新たに出現した 双極高速ジェットからの同時噴出ガス塊今井 裕, 宇野友理, 前山大地, 山口諒祐, 甘田 渓, 濱江勇希(鹿児島大学),

Ross Burns(国立天文台), Gabor Orosz (タスマニア大学),

José Francisco Gómez (スペイン高等学術研究院),

Daniel Tafoya (オンサラ天文台), Lucero Uscanga(メキシコ自治大学)

2019年度連星系・変光星研究会

＠中京大学 2019年11月30日

NESS-NROComprehensive mapping of cold circumstellar envelopes in CO /13CO J=1→0 lines

Contours: JCMT 850 μm

30 000 AU @ 300pc

Amada, Imai et al. in prep.

Water fountains Fast bipolar jets from dying stars traced by H2O masers

Image with ALMA+VLBA (Tafoya, Imai et al. in prep.)

CO J=2→1 (70 — 110 km/s) CO J=2→1 (-110 — -70 km/s) H2O masers (<90 km/s) 230 GHz dust continuum

Jet’s dynamical age: t~50 yearsPeriodic eruptions in 7 year cycle?Faster jet bullets with deceleration?

W43A

ALMA’s beam

500 AU @ 2.2 kpc

FLASHING Finest Legacy Acquisitions of SiO- and H2O-maser

Ignitions by Nobeyama Generation

Using Nobeyama 45-m telescope + Perforated frequency separation filter plate

(Okada et al. 2020, PASJ) developed by HINOTORI (Hybrid Installation Project in Nobeyama, Triple-band Oriented)

Conducted as a Backup Program during 2018 December—2019 May (~260 hours)

Towards 17(+2) water fountains and candidates 3—14 observation sessions per source Velocity resolution: 0.42 km/s (H2O) and 0.22 km/s (SiO) Velocity coverage: 1258 km/s (H2O) Follow-up VLBI target-of-opportunity observations soon after new ignitions of highest velocity H2O maser components Will be registered in M2O (maser monitoring organization)

Science goals of FLASHINGMonitoring 17 water fountains and candidates

Flux periodicity caused by stellar pulsation (1—5 years) Permanent death, evolving to a planetary nebula (~10 years) Recurrent outbursts caused by interactions in a binary system with a large eccentricity (>5 years) Line-of-sight velocity drifts caused by jet deceleration

Very long baseline time-domain radio astronomy

Before ignitions of the highest velocity H2O maser components

Imai et al. (2020, PASJ VERA Special Issue)

Systemic velocity (~50 km/s)

IRAS 18286-0959

New ignitions of the highest velocity H2O maser components

Imai et al. (2020, PASJ VERA Special Issue)

-160 -80 0 80 160 240LSR velocity [km/s]

Systemic velocity (~50 km/s)

IRAS 18286-0959

New ignitions of the highest velocity H2O maser components

Imai et al. (2020, PASJ VERA Special Issue)

-160 -80 0 80 160 240LSR velocity [km/s]

KaVA (KVN and VERA Combined Array)

target-of-opportunity follow-up

Epoch: 2019 March 4 for 6 hours

Participating telescopes: 4 VERA and 3 KVN antennas in LHCP

1Gbps recording —> Velocity coverage 1727 km/s 4096 channels —> Velocity resolution 0.42 km/s Synthesized beam: 2.1x1.4 mas, P.A.=-18 deg. 1-σ noise level: ~20 mJy/beam Maser spot identification: > 7-σ noise level

Localization of the highest velocity H2O maser components

Imai et al. (2020, PASJ VERA Special Issue)

-150

-10

0

-50

0

50

1

00

150

200

2

50LS

R ve

locity

(km

s-1)

R.A. offset (mas)

Decl.

offse

t (ma

s)-2

00

-

100

0

1

00

200

0 -100

+1a

1b2b

2a3a

3b

4b

4a5a

5b

Mapped with KaVA (KVN and VERA Combined Array)

on 2019 March 6

Highest velocity jet before deceleration

Point symmetric pattern of maser distribution in a ~3.5 year spacing

Decadal jet evolution

Imai et al. (2020, PASJ VERA Special Issue)

Clockwise precession and lobe expansion of the bipolar jet Dynamical age ~30 years New maser ignition after 2011

Short-lived (t<1 month) spots before 2011? Previous maser ignition before 2006?

Jet deceleration from 300 km/s to 110 km/s so as to mix with entrained material in ~3.5 years(?)

⇩

Velocity drift over ~10 km/s/yr!

By-product of FLASHING Watching propagation of a shock wave?

S CrB SiO v=2 J=1→0 masers

(2018 December—2019 May

2 km/s100 days

Systemic velocity VLSR~-5 km/s (Famaey et al. 2005, A&Ap, 430, 165)

By-product of FLASHING

0.15 km/s

Or watching mis-calculation of LSR velocity…… ?

AcknowledgementsVery thanks to

Nobeyama Radio Observatory (Development Proposal 4171001) Mizusawa VLBI Observatory KVN/KASI AGARC, Kagoshima University FLASHING Team

KAKENHI grant-in-aid 16H02167 (P.I. Hiroshi Imai)

NAOJ Development Program P.I. Takeshi Manabe (FY2016, FY2017)